SiS in Circumstellar Shells

Details SiS in Circumstellar Shells SiS in Circumstellar Shells

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mlrg.proc..151s&link_type=abstract

Mass Loss from Red Giants; Proceedings of the Conference, University of California, Los Angeles, CA, June 20, 21, 1984. Edited

Astronomy and Astrophysics

Astrophysics

Scientific paper

The author has observed the spectrum of SiS toward the Mira variable IRC+10216, and made a detailed model incorporating a radial SiS abundance gradient due to photodissociation by interstellar UV (Sahai, Wootten, and Clegg 1984). The sensitive search for SiS J = 7-6 and J = 6-5 lines in other carbon-rich, oxygen-rich, and S-type envelopes has revealed three new sources, CIT 6, CRL 2688 and IRC+20370, all of which are carbon-rich.

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